电邮这篇文章 Low-Mass Neutron Stars with Rotation
- 作者: Yudin A.V.1,2, Razinkova T.L.1, Blinnikov S.I.1,3
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隶属关系:
- Institute for Theoretical and Experimental Physics
- “Kurchatov Institute” National Research Center
- Kavli IPMU
- 期: 卷 45, 编号 12 (2019)
- 页面: 847-854
- 栏目: Article
- URL: https://ogarev-online.ru/1063-7737/article/view/191725
- DOI: https://doi.org/10.1134/S1063773719120077
- ID: 191725
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详细
The properties of low-mass neutron stars with rigid rotation are considered. The possible evolution paths of such stars in a close binary system with mass transfer are calculated. The properties of the gamma-ray burst GRB 170817A interpreted in terms of the stripping model, a natural ingredient of which is the explosion of a low-mass neutron star—a binary component, are briefly discussed.
作者简介
A. Yudin
Institute for Theoretical and Experimental Physics; “Kurchatov Institute” National Research Center
编辑信件的主要联系方式.
Email: yudin@itep.ru
俄罗斯联邦, ul. Bolshaya Cheremushkinskaya 25, Moscow, 117259; pl. Kurchatova 1, Moscow, 123182
T. Razinkova
Institute for Theoretical and Experimental Physics
Email: yudin@itep.ru
俄罗斯联邦, ul. Bolshaya Cheremushkinskaya 25, Moscow, 117259
S. Blinnikov
Institute for Theoretical and Experimental Physics; Kavli IPMU
Email: yudin@itep.ru
俄罗斯联邦, ul. Bolshaya Cheremushkinskaya 25, Moscow, 117259; Kashiwa
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